Gravitational fields of rotating magnetized stars

Details Gravitational fields of rotating magnetized stars Gravitational fields of rotating magnetized stars

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mvsmm.......54z&link_type=abstract

Moskovskii Universitet, Vestnik, Seriia 1 - Matematika, Mekhanika (ISSN 0579-9368), Sept.-Oct. 1989, p. 54-59. In Russian.

Statistics

Computation

Computational Astrophysics, Gravitational Fields, Magnetic Stars, Stellar Rotation, Asymptotic Methods, Potential Theory

Scientific paper

An integral equation describing the behavior of axisymmetric stationary electromagnetic and gravitational fields of sources continuously distributed on the axis of symmetry is obtained. A relationship is found between the multipole expansion at infinity and the distribution density of the sources. The behavior of gravitational fields in the near zone is described for thin elongated bodies.

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